Meridional circulation and dynamo-wave propagation

Details Meridional circulation and dynamo-wave propagation Meridional circulation and dynamo-wave propagation

Feb 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008arep...52..157p&link_type=abstract

Astronomy Reports, Volume 52, Issue 2, pp.157-163

Astronomy and Astrophysics

Astronomy

4

95.30.Qd, 96.60.Hv, 97.10.Ld, Magnetohydrodynamics And Plasmas, Electric And Magnetic Fields, Solar Magnetism, Magnetic And Electric Fields, Polarization Of Starlight

Scientific paper

The effects of meridional circulation on the solar dynamo wave are investigated in the Parker approximation using WKB techniques. The meridional circulation can substantially prolong the activity cycle; however, in the framework of the approximation considered, it cannot reverse the direction of propagation of the dynamo wave. If the circulation speed is too high, the solution is concentrated near the pole and can no longer be described in the Parker approximation.

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